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Re: [Phys-l] Simulating disturbances in a stable planetary system.



On Jan 2, 2008, at 3:06 PM, John Denker wrote:

On 01/02/2008 10:32 AM, chuck britton wrote:

How about the term 'equilibrium'?

I think that it might more clearly relate to this discussion.

Two body orbits remain in equilibrium when disturbed but are no
longer in the same 'state'.

No, you don't want to go down that rabbit-hole.

In mechanics, the terms equilibrium, stability, and damping
are well defined. The definitions are not likely to change
any time soon.

A pedagogical discussion of this, including some useful diagrams,
can be found at
http://www.av8n.com/how/htm/equilib.html

A reclining cone remains in equilibrium when disturbed but not in the
same state.

OK.

A standing cone is in equilibrium so dramatically that it is often
referred to as Stable Equilibrium.

"Drama" is not part of the definition.

It is of course more rightly seen as a Meta-Stable equilibrium when
the disturbance is comparable to the 'depth of the equilibrium well'.

The difference between stability and metastability is usually
only a matter of degree. Absolute, unconditional stability is
rare and hard to achieve.

Feynmann was certainly correct when he would scorn the
'Give it a Name and we'll Understand it'

Yeah, but the funny thing is that students still want names.
Students overestimate the importance of terminology by a
factor of 100 or so.

There *is* a cost to not knowing the terminology, as Feynman
well knew
http://www.multitran.ru/c/m.exe? a=DisplayParaSent&fname=Richard%20Feynman%5CChapter09

I like to say that ideas are primary and terminology is
secondary. Terminology is useful to the extent that it
helps us formulate and communicate the ideas.

In contrast, terminology for the sake of terminology
is a colossal waste of time.

Loosely speaking, terminology is like laboratory apparatus,
in the following sense: One of my favorite John Reppy quotes
is:
"You should never build any more apparatus than you need,
or any less."

1) In the last two days i was playing with my own planetary simulation program (one planet m<<M). Its output is not as fancy as that in I.P. (commercial Interactive Physics software) but it allows me to create disturbances that I was not able to produce in I.P. Both programs produce identical results for unperturbed motions when initial conditions are the same. That was done to check that no serious errors were made in my code.

2) My program was used with different kinds of disturbances, such a change in position (suddenly moving a planet into a position in which the fields is either stronger or weaker), or a sudden change in velocity, or both, etc. I never observed the effect which, according to JohnD, would be called "positive stability" (see the first URL above). Disturbances change trajectories, for example, a circular orbit becomes elliptical. Or an elliptical orbit becomes longer. In the absence of disturbances each orbit is persistent/durable (periodic). A motion in a state of "negative stability" (usually called unstable) could also be produced. These were cases in which the escape velocity was exceeded by the planet. On that basis one can say that a two-body planetary system is never "positively stable." The potential energy does not have a minimum, when plotted against the distance between two objects. That is why positive stability does not happen.

3) By the way, consider an elliptical trajectory and plot the distance r versus time. You will see oscillations between r(min) and r(max). The cycles repeat themselves periodically. But changes in r near the r(min) are more rapid than changes in r near r(max); the d(t) is not a sin curve. The potential energy, U, is inversely proportional to d. Thus maxima in r(t) correspond to minima in U(t), and vice versa. There is nothing profound in this. But I find it interesting.

_______________________________________________________
Ludwik Kowalski, a retired physicist
5 Horizon Road, apt. 2702, Fort Lee, NJ, 07024, USA
Also an amateur journalist at http://csam.montclair.edu/~kowalski/cf/